Nuclear Propulsion for a Manned Mission to Mars. Robert Sheldon and Rod Clark Grassmere Dynamics, LLC NSSTC, Huntsville, Alabama Apr 22, 2010. Abstract.
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Robert Sheldon and Rod Clark
Grassmere Dynamics, LLC
NSSTC, Huntsville, Alabama
Apr 22, 2010
We discuss a novel dusty-plasma fission-fragment nuclear rocket that can provide both thrust and electricity for a mission to Mars, substantially improving over the 40+ year old NERVA. It is able to achieve higher power (~5GW) than NERVA (~1GW) through its innovative dusty core that cools very efficiently by radiation. It is able to achieve higher specific impulse (~100,000s) than NERVA (~800s) or DS1 (~10,000s) by emitting fission fragments at a few percent of the speed of light where the charged dust is confined by strong magnetic and electric fields, which also transfer the thrust. It uses modern neutron moderators that are about 100 times more effective and lighter weight than NERVA, for a "wet" mass of a few tons. It can produce electricity directly from the charged fission fragments at about 85% efficiency, with less thermal radiators than the corresponding Carnot process of "nuclear-electric". The environmental impact of radioactive exhaust for starting the rocket in low-earth orbit amounts to approximately one years worth of natural C14 production, depending on space weather. And finally, it uses proven HEU or Pu reactor fuel, which other than its processing as dust, is readily available. In conclusion, this technology may have broken through the twin barriers of cost and safety, permitting astronauts a speedy transport to and timely return from Mars.
Material Isp Limitation (more=better)
Solid fuel 200-250 fuel-starved
LH2/LOX 350-450 fuel-starved
Nuclear Thermal 825-925 efficiency-starved
Gas Core Nuclear ~2,000 efficiency-starved
MHD < 5,000 energy-starved
Ion < 10,000 energy-starved
Fission Fragment ~1,000,000 fuel-starved
Matter-Antimatter ~10,000,000 fuel-starved
30-day computed w/o orbital dynamics
Fission Frag 1Ms
Fusion Frag 2Ms
1.5GW Pu239 reactor cooled with GH2 run for >30 minutes, stopped and restarted without incident at Jackass Flats NV. One version made 4.08GW for 12 minutes. Held the record almost 30 years for the highest power nuclear reactor on Earth.
-Mass (dry) = 34 ton
-Diameter = 10.5 m
-Thrust = 867 kN in vacuum
Could place men on Mars by 1985. Cancelled in 1972.
Shield shadow terminator
Power Lines, Coolant tubes
Fission Fragments have ~2MeV /nuc of energy and about 26 + charges. Rings are biassed at higher and higher + Voltage. Moving current uphill is like charging a battery. ~85% efficiency.
Collector shapes can be optimized for collecting “at rest” FF.
Coils at each end of the FF reactor control how much FF go into thrust, and how much into electricity.
Operating the nuclear reactor at max efficiency, we can adjust thrust and electricity separately.
Charged dust + plasma = a “plum pudding” Coulomb crystal, or as Cooper-pairs in BCS theory. Note surface tension & crystalline interaction.
Auburn University University of Iowa
If the dust grain is less than 1 micron, the FF escape nearly 100% without “friction”. ==> No heat.
Since we need a total amount of U235 to achieve criticality, how do we collect enough dust grains without heating them?
Arc discharge on 3μ SiO2 dust grains charges them negative. Probable charge state on dust is –10,000 e/grain.
They are trapped in a positive space-charge region adjacent to ring current. The RC is formed by -400V DC glow discharge on NIB magnet, streaming electrons ionize the air, maintain the RC. Phase-space mismatch of streaming electrons and trapped ions produces the space charge. Highly anisotropic B-field contributes as well.The Dust Trap
Black line is U235 with LiH moderator. Red line is Pu239 with C13-D moderator.Size of Critical Cloud
Concept with C13-D moderator.
35MW Fission Fragment Rocket